Table 2: Measures of the equivalent widths of the Li  I 6708 Å and H$ {\alpha }$ lines and of radial and rotational velocities for the 7 stars observed with SARG.
star Li EW H$ {\alpha }$ EW $v_{\rm rad}$ $v_{\rm rot}~\sin i$ Spectral
  Å Å km s-1 km s-1 classification
new TMC members
XEST-09-042 $0.53\pm 0.03$ $-3.2\pm 0.5$ $16.7\pm 1.0$ 31.3+2.8-2.1 K5-7 V/IV
XEST-08-003 $0.56\pm 0.05$ -2.5+0.4-0.7 $16.2\pm 1.5$ 44+4-3 K5-7 V/IV
XEST-26-062 a $0.46\pm 0.06$ $-9.0\pm 1.5$ $14.4\pm 1.1$ $18\pm 3$ M
non members
XEST-11-035 <0.03 0.76+0.15-0.06 $10.39\pm 0.25$ <4 K5 V
XEST-21-059 <0.025 $1.5\pm 0.2$ $88.10\pm 0.23$ <5 K1 IV/III
XEST-04-060 <0.025 $1.4\pm 0.2$ $19.34\pm 0.23$ <5 K1 IV/III
XEST-27-022 <0.02 $1.45\pm 0.15$ $9.13\pm 0.19$ <5 K1 IV/III
a Absolute values of the equivalent widths of the Li and H$ {\alpha }$ lines
are likely underestimated since veiling was not accounted for.


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